# -*- coding: utf-8 -*-
"""
Attitude from angular rate
==========================

Unitary quaternions [#]_ are used when representing an attitude. They can be
updated via integration of angular rate measurements of a gyroscope.

The easiest way to do so is by integrating the differential
equation for a local rotation rate :cite:p:`sola2017quaternion`.

In a kinematic system, the angular velocity :math:`\\boldsymbol\\omega` of a
rigid body at any instantaneous time is described with respect to a fixed frame
coinciding instantaneously with its body frame. Thus, this angular
velocity is *in terms of* the body frame :cite:p:`jia2024`.

Accumulating rotation over time in quaternion form is done by integrating the
differential equation of :math:`\\mathbf{q}` with a defined rotation rate.
This constant augmentation is sometimes termed the **Attitude Propagation**.

.. math::
    \\hat{\\mathbf{q}}_t = \\mathbf{q}_{t-1} + \\int_{t-1}^t\\boldsymbol\\omega\\, dt

Exact closed-form solutions of the integration are not available. Thus, an
approximation method is required. Besides, numerical methods don't give a
continuous solution for :math:`\\mathbf{q}`, but a discrete set of values can:
:math:`\\mathbf{q}_t`, :math:`n=1,2,\\dots`

In the simplest practical case, the angular rates are measured by `gyroscopes
<https://en.wikipedia.org/wiki/Gyroscope>`_, reading instantaneous angular
velocities, :math:`\\boldsymbol\\omega(t_n)
=\\begin{bmatrix}\\omega_x&\\omega_y&\\omega_z\\end{bmatrix}^T`,
in *rad/s*, at discrete times :math:`t_n = n\\Delta t` in the local sensor
frame.

The parameter :math:`\\Delta t` is called *time step* or *step size* of the
numerical integration.

Quaternion Derivative
---------------------

We start by expressing our angular velocity in quaternion form, so that we can
use the quaternion derivative to integrate it and estimate the new attitude.

An orientation (attitude) is described with a quaternion :math:`\\mathbf{q} (t)`
at a time :math:`t`, and with :math:`\\mathbf{q} (t+\\Delta t)` at a time
:math:`t+\\Delta t`. This is after a rotation change :math:`\\Delta\\mathbf{q}`
during :math:`\\Delta t` seconds is performed on the local frame
:cite:p:`jia2024`.

This rotation change about the instantaneous axis
:math:`\\mathbf{u}=\\frac{\\boldsymbol\\omega}{\\|\\boldsymbol\\omega\\|}`
through the angle :math:`\\theta=\\|\\boldsymbol\\omega\\|\\Delta t` can be
described by a quaternion too:

.. math::
    \\begin{array}{rcl}
    \\Delta\\mathbf{q} &=& \\cos\\frac{\\theta}{2} + \\mathbf{u}\\sin\\frac{\\theta}{2} \\\\
    &=& \\cos\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2} + \\frac{\\boldsymbol\\omega}{\\|\\boldsymbol\\omega\\|}\\sin\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2}
    \\end{array}

implying that :math:`\\mathbf{q}(t+\\Delta t)=\\Delta\\mathbf{qq}(t)`. To
obtain the derivative we consider :math:`\\mathbf{q} = \\mathbf{q}(t)` as the
original state at a time :math:`t`, and the difference between states as:

.. math::
    \\begin{array}{rcl}
    \\mathbf{q}(t+\\Delta t)-\\mathbf{q}(t)
    &=& \\Big(\\cos\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2} + \\frac{\\boldsymbol\\omega}{\\|\\boldsymbol\\omega\\|}\\sin\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2}\\Big)\\mathbf{q} - \\mathbf{q} \\\\
    &=& \\Big(-2\\sin^2\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{4} + \\frac{\\boldsymbol\\omega}{\\|\\boldsymbol\\omega\\|}\\sin\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2}\\Big)\\mathbf{q}
    \\end{array}

The development of the `time-derivative <https://en.wikipedia.org/wiki/Differential_calculus#Derivative>`_
of the quaternions [#]_ follows the formal definition:

.. math::
    \\begin{array}{rcl}
    \\dot{\\mathbf{q}}
    &=& \\underset{\\Delta t\\to 0}{\\mathrm{lim}} \\frac{\\mathbf{q}(t+\\Delta t)-\\mathbf{q}(t)}{\\Delta t} \\\\
    &=& \\underset{\\Delta t\\to 0}{\\mathrm{lim}} \\frac{1}{\\Delta t}\\Big(-2\\sin^2\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{4} + \\frac{\\boldsymbol\\omega}{\\|\\boldsymbol\\omega\\|}\\sin\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2}\\Big)\\mathbf{q} \\\\
    &=& \\frac{\\boldsymbol\\omega}{\\|\\boldsymbol\\omega\\|} \\underset{\\Delta t\\to 0}{\\mathrm{lim}} \\frac{1}{\\Delta t}\\sin\\big(\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2}\\big) \\mathbf{q} \\\\
    &=& \\frac{\\boldsymbol\\omega}{\\|\\boldsymbol\\omega\\|} \\frac{d}{dt} \\sin\\big(\\frac{\\|\\boldsymbol\\omega\\|}{2}t\\big) \\Big || _{t=0} \\; \\mathbf{q} \\\\
    &=& \\frac{1}{2}\\boldsymbol\\omega \\mathbf{q} \\\\
    &=& \\frac{1}{2}
    \\begin{bmatrix}
    -\\omega_x q_x -\\omega_y q_y - \\omega_z q_z\\\\
    \\omega_x q_w + \\omega_z q_y - \\omega_y q_z\\\\
    \\omega_y q_w - \\omega_z q_x + \\omega_x q_z\\\\
    \\omega_z q_w + \\omega_y q_x - \\omega_x q_y
    \\end{bmatrix}
    \\end{array}

.. warning::
    The product between the angular velocity :math:`\\boldsymbol\\omega\\in\\mathbb{R}^3`
    and the quaternion :math:`\\mathbf{q}\\in\\mathbb{H}^4` is done by
    representing the former as a pure quaternion :math:`\\boldsymbol\\omega=
    \\begin{bmatrix}0 & \\omega_x & \\omega_y & \\omega_z\\end{bmatrix}\\in\\mathbb{H}^4`,
    so that a `Hamilton Product <https://en.wikipedia.org/wiki/Quaternion#Hamilton_product>`_
    can be applied.

Defining the omega operator as

.. math::
    \\boldsymbol\\Omega(\\boldsymbol\\omega) =
    \\begin{bmatrix}0 & -\\boldsymbol\\omega^T \\\\ \\boldsymbol\\omega & -\\lfloor\\boldsymbol\\omega\\rfloor_\\times\\end{bmatrix} =
    \\begin{bmatrix}
    0 & -\\omega_x & -\\omega_y & -\\omega_z \\\\
    \\omega_x & 0 & \\omega_z & -\\omega_y \\\\
    \\omega_y & -\\omega_z & 0 & \\omega_x \\\\
    \\omega_z & \\omega_y & -\\omega_x & 0
    \\end{bmatrix}

.. note::
    The expression :math:`\\lfloor\\mathbf{x}\\rfloor_\\times` expands a vector
    :math:`\\mathbf{x}\\in\\mathbb{R}^3` into a :math:`3\\times 3`
    `skew-symmetric matrix <https://en.wikipedia.org/wiki/Skew-symmetric_matrix>`_:

    .. math::
        \\lfloor\\mathbf{x}\\rfloor_\\times =
        \\begin{bmatrix} 0 & -x_2 & x_1 \\\\ x_2 & 0 & -x_0 \\\\ -x_1 & x_0 & 0\\end{bmatrix}

we get an equivalent matrix expression for the derivative:

.. math::
    \\dot{\\mathbf{q}} = \\frac{1}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\mathbf{q}

This definition does **not** require a Hamilton product and the Omega operator
can be used as a common matrix to multiply with the quaternion as any other
linear operation.

Quaternion Integration
----------------------

First, let's remember the definition of a vector or `matrix exponential
<https://en.wikipedia.org/wiki/Matrix_exponential>`_ as a power series:

.. math::
    e^\\mathbf{X} = \\sum_{k=0}^\\infty \\frac{1}{k!} \\mathbf{X}^k

Letting :math:`\\mathbf{v}=\\mathbf{u}\\theta` be the **rotation vector**,
representing a rotation of :math:`\\theta` radians around the unitary axis
:math:`\\mathbf{u}=\\begin{bmatrix}u_x & u_y & u_z\\end{bmatrix}^T`, we can
get its exponential series as:

.. math::
    e^\\mathbf{v} = e^{\\mathbf{u}\\theta} = \\Big(1 - \\frac{\\theta^2}{2!} + \\frac{\\theta^4}{4!} + \\cdots\\Big)
    + \\Big(\\mathbf{u}\\theta - \\frac{\\mathbf{u}\\theta^3}{3!} + \\frac{\\mathbf{u}\\theta^5}{5!} + \\cdots\\Big)

We recognize the power-series expansion of `Euler's formula
<https://en.wikipedia.org/wiki/Euler%27s_formula#Using_power_series>`_, which
helps to map the quaternion :math:`\\mathbf{q}` from a rotation vector
:math:`\\mathbf{v}`. This **exponential map** :cite:p:`sola2017quaternion` is formerly defined as:

.. math::
    \\mathbf{q} = e^\\mathbf{v} =
    \\begin{bmatrix}\\cos\\frac{\\theta}{2} \\\\
    \\mathbf{u}\\sin\\frac{\\theta}{2}\\end{bmatrix}

Assuming the gyroscope data is sampled at a fixed rate and that the angular
velocity vector, :math:`\\boldsymbol\\omega`, in local body coordinates is
constant over the sampling interval :math:`\\Delta t`, we can alternatively
integrate :math:`\\dot{\\mathbf{q}}` to obtain:

.. math::
    \\mathbf{q}_{t+1} = e^{\\frac{1}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\Delta t}\\mathbf{q}_t

Using the `Euler-Rodrigues rotation formula
<https://en.wikipedia.org/wiki/Quaternions_and_spatial_rotation#Using_quaternion_as_rotations>`_
and the exponential map from above we find a **closed-form solution**
:cite:p:`spence1978`:

.. math::
    \\mathbf{q}_{t+1} =
    \\Bigg[
    \\cos\\Big(\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2}\\Big)\\mathbf{I}_4 +
    \\frac{1}{\\|\\boldsymbol\\omega\\|}\\sin\\Big(\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2}\\Big)\\boldsymbol\\Omega(\\boldsymbol\\omega)
    \\Bigg]\\mathbf{q}_t

where :math:`\\mathbf{I}_4` is a :math:`4\\times 4` Identity matrix. The large
term inside the brackets, multiplying :math:`\\mathbf{q}_t`, is an orthogonal
rotation retaining the normalization of the propagated attitude quaternions.
Thus, it is not necessary to normalize :math:`\\mathbf{q}_{t+1}`, but it is
highly recommended to do so in order to avoid any `round-off errors
<https://en.wikipedia.org/wiki/Round-off_error>`_ inherent to all computers.

We can stop here and use this closed-form solution to update the quaternion,
but it cannot be used in a linear system. For that, we need to linearize the
quaternion update equation.

Quaternion Linearization
------------------------

Now we develop an :math:`n^{th}`-order polynomial linearization method built
from `Taylor series <https://en.wikipedia.org/wiki/Taylor_series>`_ of
:math:`\\mathbf{q}(t+\\Delta t)` around the time :math:`t` for the quaternion:

.. math::
    \\mathbf{q}_{t+1} = \\mathbf{q}_t + \\dot{\\mathbf{q}}_t\\Delta t +
    \\frac{1}{2!}\\ddot{\\mathbf{q}}_t\\Delta t^2 +
    \\frac{1}{3!}\\dddot{\\mathbf{q}}_t\\Delta t^3 + \\cdots

Using the definition of :math:`\\dot{\\mathbf{q}}` the new orientation
:math:`\\mathbf{q}_{t+1}` is written as :cite:p:`spence1978`:

.. math::
    \\begin{array}{rcl}
    \\mathbf{q}_{t+1} &=& \\Bigg[\\mathbf{I}_4 + \\frac{1}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\Delta t +
    \\frac{1}{2!}\\Big(\\frac{1}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\Delta t\\Big)^2 +
    \\frac{1}{3!}\\Big(\\frac{1}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\Delta t\\Big)^3 + \\cdots\\Bigg]\\mathbf{q}_t \\\\
    && \\qquad{} + \\frac{1}{4}\\dot{\\boldsymbol\\Omega}(\\boldsymbol\\omega)\\Delta t^2\\mathbf{q}_t
    + \\Big[\\frac{1}{12}\\dot{\\boldsymbol\\Omega}(\\boldsymbol\\omega)\\boldsymbol\\Omega(\\boldsymbol\\omega)
    + \\frac{1}{24}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\dot{\\boldsymbol\\Omega}(\\boldsymbol\\omega)\\Big]\\Delta t^3\\mathbf{q}_t
    + \\frac{1}{12}\\ddot{\\boldsymbol\\Omega}(\\boldsymbol\\omega)\\Delta t^3\\mathbf{q}_t
    + \\cdots
    \\end{array}

Assuming the angular rate is constant over the period :math:`[t, t+1]`, we have
:math:`\\dot{\\boldsymbol\\omega}=0`, and we can prescind from the derivatives
of :math:`\\boldsymbol\\Omega` reducing the series to:

.. math::
    \\mathbf{q}_{t+1} = \\Bigg[\\mathbf{I}_4 + \\frac{1}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\Delta t +
    \\frac{1}{2!}\\Big(\\frac{1}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\Delta t\\Big)^2 +
    \\frac{1}{3!}\\Big(\\frac{1}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\Delta t\\Big)^3 + \\cdots\\Bigg]\\mathbf{q}_t

Notice the series for :math:`\\mathbf{q}_{t+1}` also follows the form of the
matrix exponential:

.. math::
    e^{\\frac{\\Delta t}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)} =
    \\sum_{k=0}^\\infty \\frac{1}{k!} \\Big(\\frac{\\Delta t}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\Big)^k

The error of the approximation vanishes rapidly at higher orders (:math:`k \\to
0`), or when the time step :math:`\\Delta t \\to 0`. The more terms we have,
the better our approximation should be, assuming the sensor signals are
unbiased and noiseless, with the downside of a big computational demand.

For our purpose a truncation up to the second term, making it of first order
(:math:`k=1`), is implemented.

.. math::
    \\mathbf{q}_{t+1} = \\Bigg[\\mathbf{I}_4 + \\frac{1}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\Delta t\\Bigg]\\mathbf{q}_t

Two good reasons for this truncation are:

- Simple architectures (like embedded systems) avoid the burden of the heavy
  computation, and still achieve fairly good results.
- If the sensor signals are not properly filtered and corrected, the estimation
  will not converge to a good result, and even worsening it at higher orders.

The resulting quaternion must be normalized to operate as a versor, and to
represent a valid orientation.

.. math::
    \\mathbf{q}_{t+1} \\gets \\frac{\\mathbf{q}_{t+1}}{\\|\\mathbf{q}_{t+1}\\|}

Numerical Integration based on Runge-Kutta methods can be employed to increase
the accuracy, and are shown to be more effective. See :cite:p:`sola2017quaternion`
and :cite:p:`zhao2013` for a comparison of the different methods, their
accuracy, and their computational load.

Footnotes
---------

.. [#] A vector :math:`\\mathbf{x}` is unitary if its norm is equal to one:
    :math:`\\|\\mathbf{x}\\|=1`.
.. [#] The successive derivatives of :math:`\\mathbf{q}_n` are obtained by
    repeatedly applying the expression of the quaternion derivative,
    with :math:`\\ddot{\\boldsymbol\\omega}=0`.

    .. math::
        \\begin{array}{rcl}
        \\dot{\\mathbf{q}}_n &=& \\frac{1}{2}\\mathbf{q}_n\\boldsymbol\\omega_n \\\\
        \\ddot{\\mathbf{q}}_n &=& \\frac{1}{4}\\mathbf{q}_n\\boldsymbol\\omega^2_n + \\frac{1}{2}\\mathbf{q}_n\\dot{\\boldsymbol\\omega} \\\\
        \\dddot{\\mathbf{q}}_n &=& \\frac{1}{2^3}\\mathbf{q}_n\\boldsymbol\\omega^3_n + \\frac{1}{4}\\mathbf{q}_n\\dot{\\boldsymbol\\omega}\\boldsymbol\\omega_n + \\frac{1}{2}\\mathbf{q}\\boldsymbol\\omega_n\\dot{\\boldsymbol\\omega} \\\\
        \\mathbf{q}^{i\\geq 4}_n &=& \\frac{1}{2^i}\\mathbf{q}_n\\boldsymbol\\omega^i_n + \\cdots
        \\end{array}

    where all products and the powers of :math:`\\boldsymbol\\omega` are
    interpreted in terms of the quaternion product.

"""

import numpy as np
from ..utils.core import _assert_numerical_iterable
from ..common.quaternion import QuaternionArray
from ..common.dcm import DCM

class AngularRate:
    """
    Quaternion update by integrating measured angular velocities.

    All estimated quaternions are stored in the attribute ``Q`` as a
    :class:`numpy.ndarray` of shape *(N, 4)*, where *N* is the number of
    estimated attitudes. The first row is the initial attitude, and the last
    row is the final attitude.

    Parameters
    ----------
    gyr : numpy.ndarray, default: None
        N-by-3 array with measurements of angular velocity in rad/s.
    q0 : numpy.ndarray
        Initial orientation, as a versor (normalized quaternion).
    frequency : float, default: 100.0
        Sampling frequency in Herz.
    Dt : float, default: 0.01
        Sampling step in seconds. Inverse of sampling frequency. Not required
        if ``frequency`` value is given.
    method : str, default: ``'closed'``
        Estimation method to use. Options are: ``'series'``, ``'closed'``, or
        ``'integration'``. The option ``'integration'`` is a simple numerical
        integration of the angular velocity as roll-pitch-yaw angles.
    order : int
        Truncation order, if method ``'series'`` is used.
    representation : str, default: ``'quaternion'``
        Attitude representation. Options are ``'quaternion'``, ``'angles'`` or
        ``'rotmat'``.

    Examples
    --------
    >>> gyro_data.shape             # NumPy arrays with gyroscope data in rad/s
    (1000, 3)
    >>> from ahrs.filters import AngularRate
    >>> angular_rate = AngularRate(gyr=gyro_data)
    >>> angular_rate.Q
    array([[ 1.00000000e+00,  0.00000000e+00,  0.00000000e+00,  0.00000000e+00],
           [ 9.99999993e-01,  2.36511228e-06, -1.12991334e-04,  4.28771947e-05],
           [ 9.99999967e-01,  1.77775173e-05, -2.43529706e-04,  8.33144162e-05],
           ...,
           [-0.92576208, -0.23633121,  0.19738534, -0.2194337 ],
           [-0.92547793, -0.23388968,  0.19889139, -0.22187479],
           [-0.92504595, -0.23174096,  0.20086376, -0.22414251]])
    >>> angular_rate.Q.shape        # Estimated attitudes as Quaternions
    (1000, 4)

    The estimation of each attitude is built upon the previous attitude. This
    estimator sets the initial attitude equal to the unit quaternion
    ``[1.0, 0.0, 0.0, 0.0]`` by default, because we cannot obtain the first
    orientation with gyroscopes only.

    **Initial Values**

    We can use the class :class:`.Tilt` to estimate the initial attitude with a
    simple measurement of a tri-axial accelerometer:

    >>> from ahrs.filter import Tilt
    >>> tilt = Tilt()
    >>> q_initial = tilt.estimate(acc=acc_sample)  # One tridimensional sample suffices
    >>> angular_rate = AngularRate(gyr=gyro_data, q0=q_initial)
    >>> angular_rate.Q
    array([[ 0.77547502,  0.6312126 ,  0.01121595, -0.00912944],
           [ 0.77547518,  0.63121388,  0.01110125, -0.00916754],
           [ 0.77546726,  0.63122508,  0.01097435, -0.00921875],
           ...,
           [-0.92576208, -0.23633121,  0.19738534, -0.2194337 ],
           [-0.92547793, -0.23388968,  0.19889139, -0.22187479],
           [-0.92504595, -0.23174096,  0.20086376, -0.22414251]])

    :class:`.Tilt` can also use a magnetometer to improve the estimation
    with the heading orientation.

    >>> q_initial = tilt.estimate(acc=acc_sample, mag=mag_sample)
    >>> angular_rate = AngularRate(gyr=gyro_data, q0=q_initial)
    >>> angular_rate.Q
    array([[ 0.66475674,  0.55050651, -0.30902706, -0.39942875],
           [ 0.66473764,  0.5504497 , -0.30912672, -0.39946172],
           [ 0.66470495,  0.55039529, -0.30924191, -0.39950193],
           ...,
           [-0.90988476, -0.10433118,  0.28970402,  0.27802214],
           [-0.91087203, -0.1014633 ,  0.28977124,  0.2757716 ],
           [-0.91164416, -0.09861271,  0.2903888 ,  0.27359606]])

    """
    def __init__(self, gyr: np.ndarray = None, q0: np.ndarray = None, frequency: float = 100.0, order: int = 1, **kw):
        self.gyr: np.ndarray = gyr
        self.q0: np.ndarray = q0 if q0 is not None else np.array([1.0, 0.0, 0.0, 0.0])
        self.frequency: float = frequency
        self.order: int = order
        self.method: str = kw.get('method', 'closed')
        self.representation: str = kw.get('representation', 'quaternion')
        self.Dt: float = kw.get('Dt', 1.0/self.frequency)
        if self.gyr is not None:
            if self.method.lower() == 'integration':
                self.W = self.integrate_angular_positions(self.gyr, dt=self.Dt)
            self.Q = self._compute_all()

    def _compute_all(self):
        """Estimate all quaternions with given sensor values."""
        if self.method.lower() == 'integration':
            return self.integrate_angular_positions(self.gyr, dt=self.Dt)
        num_samples = len(self.gyr)
        Q = np.zeros((num_samples, 4))
        Q[0] = self.q0
        for t in range(1, num_samples):
            Q[t] = self.update(Q[t-1], self.gyr[t], method=self.method, order=self.order)
        return Q

    def integrate_angular_positions(self, gyr: np.ndarray, dt: float = None) -> np.ndarray:
        """
        Integrate angular positions :math:`\\mathbf{\\theta}` from
        instantaneous angular rates :math:`\\mathbf{\\omega}` at a time
        :math:`t` with a given time step :math:`\\Delta t`:

        .. math::
            \\mathbf{\\theta}_{t+1} = \\mathbf{\\theta}_t + \\mathbf{\\omega}_t \\Delta t

        Given the three main roll-pitch-yaw angles, it simply integrates them
        with a cumulative sum, and returns the tri-axial angular positions.

        This method does not play a central role in this estimator, but can be
        used to obtain another reference to compare the results to.

        Calling this method is equivalent to calling::

            >>> angular_positions = numpy.cumsum(gyr * dt, axis=0)

        Parameters
        ----------
        gyr : array_like
            Angular rates, in rad/s.
        dt : float, optional
            Time step, in seconds. If not given, the time step is set to
            :math:`1/f_s`, where :math:`f_s` is the sampling frequency, which
            is defined as ``100`` Hz by default.

        Returns
        -------
        theta : numpy.ndarray
            Tri-axial angular positions, in rad.
        """
        _assert_numerical_iterable(gyr, 'gyr')
        if self.representation.lower() not in ['quaternion', 'angles', 'rotmat']:
            raise ValueError(f"Representation must be 'quaternion', 'angles' or 'rotmat'. Got '{self.representation}' instead.")
        if dt is None:
            dt = self.Dt
        if not isinstance(dt, (int, float)):
            raise TypeError(f"dt must be a float or an integer. Got {type(dt)} instead.")
        # Angular velocity integration --> Angular position
        angular_positions = np.cumsum(gyr * dt, axis=0)
        # Return angular positions in the desired representation
        if self.representation.lower() == 'quaternion':
            return QuaternionArray().from_rpy(angular_positions)
        if self.representation.lower() == 'rotmat':
            return DCM().from_quaternion(QuaternionArray().from_rpy(angular_positions))
        return np.unwrap(angular_positions, axis=0)

    def update(self, q: np.ndarray, gyr: np.ndarray, method: str = 'closed', order: int = 1, dt: float = None) -> np.ndarray:
        """
        Update the quaternion estimation

        Estimate quaternion :math:`\\mathbf{q}_{t+1}` from given a-priori
        quaternion :math:`\\mathbf{q}_t` with a measured instantaneous angular
        rate :math:`\\mathbf{\\omega}`.

        If ``method='closed'``, the new orienation is computed with the
        closed-form solution:

        .. math::
            \\mathbf{q}_{t+1} =
            \\Bigg[
            \\cos\\Big(\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2}\\Big)\\mathbf{I}_4 +
            \\frac{1}{\\|\\boldsymbol\\omega\\|}\\sin\\Big(\\frac{\\|\\boldsymbol\\omega\\|\\Delta t}{2}\\Big)\\boldsymbol\\Omega(\\boldsymbol\\omega)
            \\Bigg]\\mathbf{q}_t

        If ``method='series'``, it is computed with a series of the form:

        .. math::
            \\mathbf{q}_{t+1} =
            \\Bigg[\\sum_{k=0}^\\infty \\frac{1}{k!} \\Big(\\frac{\\Delta t}{2}\\boldsymbol\\Omega(\\boldsymbol\\omega)\\Big)^k\\Bigg]\\mathbf{q}_t

        where the order :math:`k` in the series has to be set as non-negative
        integer in the parameter ``order``. By default it is set equal to 1.

        Parameters
        ----------
        q : numpy.ndarray
            A-priori quaternion.
        gyr : numpy.ndarray
            Array with triaxial measurements of angular velocity in rad/s.
        method : str, default: ``'closed'``
            Estimation method to use. Options are: ``'series'`` or ``'closed'``.
        order : int
            Truncation order, if method ``'series'`` is used.
        dt : float, default: None
            Time step, in seconds, between consecutive Quaternions.

        Returns
        -------
        q : numpy.ndarray
            Estimated quaternion.

        Examples
        --------
        >>> from ahrs.filters import AngularRate
        >>> gyro_data.shape
        (1000, 3)
        >>> num_samples = gyro_data.shape[0]
        >>> Q = np.zeros((num_samples, 4))      # Allocation of quaternions
        >>> Q[0] = [1.0, 0.0, 0.0, 0.0]         # Initial attitude as a quaternion
        >>> angular_rate = AngularRate()
        >>> for t in range(1, num_samples):
        ...     Q[t] = angular_rate.update(Q[t-1], gyro_data[t])
        ...
        >>> Q
        array([[ 1.00000000e+00,  0.00000000e+00,  0.00000000e+00,  0.00000000e+00],
               [ 9.99999993e-01,  2.36511228e-06, -1.12991334e-04,  4.28771947e-05],
               [ 9.99999967e-01,  1.77775173e-05, -2.43529706e-04,  8.33144162e-05],
               ...,
               [-0.92576208, -0.23633121,  0.19738534, -0.2194337 ],
               [-0.92547793, -0.23388968,  0.19889139, -0.22187479],
               [-0.92504595, -0.23174096,  0.20086376, -0.22414251]])

        """
        dt = self.Dt if dt is None else dt
        if method.lower() not in ['series', 'closed']:
            raise ValueError(f"Invalid method '{method}'. Try 'series' or 'closed'")
        q = np.copy(q)
        if gyr is None or not np.linalg.norm(gyr)>0:
            return q
        Omega = np.array([
            [   0.0, -gyr[0], -gyr[1], -gyr[2]],
            [gyr[0],     0.0,  gyr[2], -gyr[1]],
            [gyr[1], -gyr[2],     0.0,  gyr[0]],
            [gyr[2],  gyr[1], -gyr[0],     0.0]])
        if method.lower() == 'closed':
            w = np.linalg.norm(gyr)
            A = np.cos(w*dt/2.0)*np.eye(4) + np.sin(w*dt/2.0)*Omega/w
        else:
            if order < 0:
                raise ValueError(f"The order must be an int equal to or greater than 0. Got {order}")
            S = 0.5 * dt * Omega
            A = np.identity(4)
            for i in range(1, order+1):
                A += S**i / np.math.factorial(i)
        q = A @ q
        return q / np.linalg.norm(q)
